Search arXiv⌕ Search

arXiv · 2610.28660

Recovering What Breaks in a Trapped-Ion Quantum Simulation of a Lattice Gauge Theory

Abstract

A recent trapped-ion experiment realised a lattice gauge theory with the gauge field in the internal states of the ions and bosonic matter in their vibrations. We showed earlier that its noise damage can be predicted. Here, we show that most of it can be undone. The conservation law of the theory is a parity of each vibrational mode, which heating flips, so a heating event leaves a mark that can be read without disturbing the physics. We keep only the runs in which this mark never changed. With equal heating rates and continuous monitoring, the kept runs reproduce the heating-free dynamics exactly, with a closed-form yield. Reading the mark at finite intervals introduces a small bias linear in the interval, which we derive and bound. At the reported rates, a single final check removes most of the heating and preparation damage while accepting eight runs out of ten.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Hassan Ugail. 2026-10-12. Recovering What Breaks in a Trapped-Ion Quantum Simulation of a Lattice Gauge Theory. https://arxiv.org/abs/2610.28660

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

A Machine Learning Approach to Finslerian Cosmological Dark Energy Model

Modified extensions of the standard cosmological models often introduce complex parameter degeneracies that severely impact sampling convergence of the parameter space while analyzing the model observationally. In this work, we present an accelerated Bayesian inference technique using a Heteroscedastic Deep Ensemble with Monte Carlo Dropout incorporating distance-gated local residual corrections to emulate complex likelihood surfaces and avoid extrapolation beyond the trained region. We demonstrate this methodology on a unified dark energy cosmological model equipped with Finsler geometry. The model is studied using the recent observational datasets, including Cosmic Chronometers (CC), Pantheon$+$SH$0$ES, and DESI DR$2$ BAO measurements. While the conventional sampling procedure struggles with slow mixing of parameter chains ($τ_{max}=1578.3$), the neural network, specially trained densely in high likelihood regions, yields converged and highly resolved posterior distributions of the model parameters without significantly compromising the minimum chi-square value. We further discuss the results for physical inferences and also compare the present dark energy model with $Λ\text{CDM}$ statistically using AIC and BIC.

physics.gen-ph↗

Sweep-Direction-Dependent Level-Attraction- and Level-Repulsion-Like Signatures in a Twisted, Helically Corrugated Microwave Resonator

We investigate photon--photon interactions in a mechanically tunable, helically corrugated rectangular microwave resonator. Mechanical twisting modifies the electromagnetic helicity and resonant frequencies of the supported modes, allowing pairs of electromagnetic modes to be tuned into near-degeneracy. Transmission magnitude and phase measurements reveal two distinct responses: a level-attraction-like response characterised by converging antiresonances and a sharp phase variation appearing as a $2π$ discontinuity in the wrapped transmission phase, and a level-repulsion-like response characterised by an anticrossing-like transmission feature. For the mode-interaction regions investigated, reversing the twist sweep direction interchanges these responses. We discuss mechanical hysteresis and changes in electromagnetic backscattering and modal interference as possible origins of this behaviour. These observations suggest a potential route towards microwave devices with mechanically switchable level-attraction-like and level-repulsion-like transmission responses.

physics.gen-ph↗

Gravitational Redshift of Light and the Heisenberg Uncertainty Principle

Empirical observations together with theoretical analyses are being used to argue that the classical phenomenon of gravitational redshift -- namely, the redshift of light in a static gravitational potential -- may be in tension with the Heisenberg uncertainty principle. In particular, in the Pound-Rebka experiment, the emitter-absorber pair interact with each other by exchanging a Mossbauer photon, a process that is fully describable within quantum mechanics but how the photon interacts with the spacetime metric remains unclear. Since the uncertainty principle is incompatible with local realism, as per general relativity, we propose to study continuous-variable photonic entanglement within the Einstein-Podolsky-Rosen (EPR) framework in a weak gravitational field. We outline a thought experiment, realizable on the surface of the Earth, that could shed further light on this problematic seamline between general relativity and quantum mechanics in the weak-field regime.

physics.gen-ph↗